CARMA Large Area Star Formation Survey: Project Overview with Analysis of Dense Gas Structure and Kinematics in Barnard 1
arXiv:1409.1233 · doi:10.1088/0004-637X/794/2/165
Abstract
We present details of the CARMA Large Area Star Formation Survey (CLASSy), while focusing on observations of Barnard 1. CLASSy is a CARMA Key Project that spectrally imaged N2H+, HCO+, and HCN (J=1-0 transitions) across over 800 square arcminutes of the Perseus and Serpens Molecular Clouds. The observations have angular resolution near 7" and spectral resolution near 0.16 km/s. We imaged ~150 square arcminutes of Barnard 1, focusing on the main core, and the B1 Ridge and clumps to its southwest. N2H+ shows the strongest emission, with morphology similar to cool dust in the region, while HCO+ and HCN trace several molecular outflows from a collection of protostars in the main core. We identify a range of kinematic complexity, with N2H+ velocity dispersions ranging from ~0.05-0.50 km/s across the field. Simultaneous continuum mapping at 3 mm reveals six compact object detections, three of which are new detections. A new non-binary dendrogram algorithm is used to analyze dense gas structures in the N2H+ position-position-velocity (PPV) cube. The projected sizes of dendrogram-identified structures range from about 0.01-0.34 pc. Size-linewidth relations using those structures show that non-thermal line-of-sight velocity dispersion varies weakly with projected size, while rms variation in the centroid velocity rises steeply with projected size. Comparing these relations, we propose that all dense gas structures in Barnard 1 have comparable depths into the sky, around 0.1-0.2 pc; this suggests that over-dense, parsec-scale regions within molecular clouds are better described as flattened structures rather than spherical collections of gas. Science-ready PPV cubes for Barnard 1 molecular emission are available for download.
Accepted to The Astrophysical Journal (ApJ), 51 pages, 27 figures (some with reduced resolution in this preprint); Project website is at http://carma.astro.umd.edu/classy
References in corpus (11)
- Theory of Star Formation
- Cold Dark Clouds: The Initial Conditions for Star Formation
- Structural Analysis of Molecular Clouds: Dendrograms
- Bias-free Measurement of Giant Molecular Cloud Properties
- The Large and Small Scale Structures of Dust in the Star-Forming Perseus Molecular Cloud
- An Ammonia Spectral Atlas of Dense Cores in Perseus
- Current Star Formation in the Perseus Molecular Cloud: Constraints from Unbiased Submillimeter and Mid-Infrared Surveys
- Formation of Magnetized Prestellar Cores with Ambipolar Diffusion and Turbulence
- CARMA Large Area Star Formation Survey: Observational Analysis of Filaments in the Serpens South Molecular Cloud
- The rotating molecular core and precessing outflow of the young stellar object Barnard 1c
- Outflow - Core Interaction in Barnard 1
Cited by in corpus (22)
- CARMA Large Area Star Formation Survey: Structure and Kinematics of Dense Gas in Serpens Main
- Self-gravitating Filament Formation from Shocked Flows: Velocity Gradients across Filaments
- The fragmentation and stability of hierarchical structure in Serpens South
- A cold accretion flow onto one component of a multiple protostellar system
- Magnetic field properties in star formation: a review of their analysis methods and interpretation
- ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions-IX. A pilot study towards IRDC G034.43+00.24 on multi-scale structures and gas kinematics
- ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XII: Fragmentation and multi-scale gas kinematics in protoclusters G12.42+0.50 and G19.88-0.53
- Connecting the Scales: Large Area High-resolution Ammonia Mapping of NGC 1333
- The VLA Nascent Disk And Multiplicity Survey of Perseus Protostars (VANDAM). III. Extended Radio Emission from Protostars in Perseus
- The Davis-Chandrasekhar-Fermi Method Revisited
- CARMA Large Area Star Formation Survey: Dense Gas in the Young L1451 Region of Perseus
- The CARMA 3mm Survey of the Inner of the Central Molecular Zone
- ALMA-IMF XIII: NH kinematic analysis on the intermediate protocluster G353.41
- Can we observe the ion-neutral drift velocity in prestellar cores?
- On the evolution of the observed Mass-to-Length relationship for star-forming filaments
- TIMES I: a Systematic Observation in Multiple Molecular Lines Toward the Orion A and Ophiuchus Clouds
- ALMA-IMF XVIII: The assembly of a star cluster: Dense NH (1-0) kinematics in the massive G351.77 protocluster
- No impact of core-scale magnetic field, turbulence, or velocity gradient on sizes of protostellar disks in Orion A
- Predictions for Observing Protostellar Outflows with ALMA
- The Hierarchical Dynamical State of Molecular Gas from 3 to 300 pc in NGC 253
- The factors that influence protostellar multiplicity II. Gas temperature and mass in Perseus with APEX
- ALMA-IMF VIII -- Combination of Interferometric Continuum Images with Single-Dish Surveys and Structural Analysis of Six Protoclusters